Using the Hapke Rough Reflectance Factor for Calibration of Atmospheric Emissions at Mercury and the Moon

Details Using the Hapke Rough Reflectance Factor for Calibration of Atmospheric Emissions at Mercury and the Moon Using the Hapke Rough Reflectance Factor for Calibration of Atmospheric Emissions at Mercury and the Moon

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002assl..278...37h&link_type=abstract

Solar System Remote Sensing, p. 37

Computer Science

Emission Spectra, Mercury Atmosphere, Lunar Atmosphere, Atmospheric Composition, Calibrating, Sodium, Potassium, Mercury (Planet), Moon

Scientific paper

Emission lines of atmospheric constituents of the Moon and Mercury (especially sodium and potassium) must be absolutely calibrated before the abundances can be obtained. It is convenient to use the intensity of the surface at an adjacent wavelength as the standard, and to use Hapke theory to obtain this intensity. This procedure and some of its pitfalls are discussed here.

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